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2
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0004266550
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edited by E. Akkermans, G. Montambaux, J.-L. Pichard, and J. Zinn-Justin, North-Holland, Amsterdam
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B.L. Altshuler and B.D. Simons, in Mesoscopic Quantum Physics, edited by E. Akkermans, G. Montambaux, J.-L. Pichard, and J. Zinn-Justin (North-Holland, Amsterdam, 1995).
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(1995)
Mesoscopic Quantum Physics
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Altshuler, B.L.1
Simons, B.D.2
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9
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4244182883
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J.A. Folk, S.R. Patel, K.M. Birnbaum, C.M. Marcus, C.I. Duruöz, and J.S. Harris, Jr., Phys. Rev. Lett. 86, 2102 (2001).
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(2001)
Phys. Rev. Lett.
, vol.86
, pp. 2102
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Folk, J.A.1
Patel, S.R.2
Birnbaum, K.M.3
Marcus, C.M.4
Duruöz, C.I.5
Harris, J.S.6
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13
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4243655096
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B.I. Halperin, A. Stern, Y. Oreg, J.N.H.J. Cremers, J.A. Folk, and C.M. Marcus, Phys. Rev. Lett. 86, 2106 (2001).
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(2001)
Phys. Rev. Lett.
, vol.86
, pp. 2106
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Halperin, B.I.1
Stern, A.2
Oreg, Y.3
Cremers, J.N.H.J.4
Folk, J.A.5
Marcus, C.M.6
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15
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85038287378
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The Hamiltonian (1) is for a two-dimensional electron gas formed parallel to the (001) plane of GaAs. The x and y coordinates are defined along axes with crystallographic directions [110] and (formula presented), in the spin-orbit Hamiltonian (notation of Ref. 11), one has (formula presented) (formula presented)
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The Hamiltonian (1) is for a two-dimensional electron gas formed parallel to the (001) plane of GaAs. The x and y coordinates are defined along axes with crystallographic directions [110] and (formula presented). In terms of the rates (formula presented) and (formula presented) for the Rashba and Dresselhaus terms in the spin-orbit Hamiltonian (notation of Ref. 11), one has (formula presented) (formula presented).
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In terms of the rates (formula presented) and (formula presented) for the Rashba and Dresselhaus terms
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17
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85038286094
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with a characteristic time that is a factor (formula presented) larger than the time scale (formula presented) characteristic of the perturbation with unitary symmetry, see Ref. 12
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A small symplectic perturbation of the Hamiltonian remains, with a characteristic time that is a factor (formula presented) larger than the time scale (formula presented) characteristic of the perturbation with unitary symmetry, see Ref. 12.
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A small symplectic perturbation of the Hamiltonian remains
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18
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0000281909
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J.P. Lu, J.B. Yau, S.P. Shukla, M. Shayegan, L. Wissinger, U. Rössler, and R. Winkler, Phys. Rev. Lett. 81, 1282 (1998).
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(1998)
Phys. Rev. Lett.
, vol.81
, pp. 1282
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Lu, J.P.1
Yau, J.B.2
Shukla, S.P.3
Shayegan, M.4
Wissinger, L.5
Rössler, U.6
Winkler, R.7
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19
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85038272508
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private communication
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C.M. Marcus (private communication).
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Marcus, C.M.1
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24
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85038308258
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P.W. Brouwer K.M. Frahm C.W.J. Beenakker.
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P.W. Brouwer K.M. Frahm C.W.J. Beenakker.
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25
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85038292189
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We assume that the momentum matrix elements multiplying (formula presented) and (formula presented) in the spin-orbit Hamiltonian (1) are equal and independently distributed
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We assume that the momentum matrix elements multiplying (formula presented) and (formula presented) in the spin-orbit Hamiltonian (1) are equal and independently distributed. This is correct when (formula presented) in Eq. (1) and the quantum dot is roughly circular.
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This is correct when (formula presented) in Eq. (1) and the quantum dot is roughly circular
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26
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0001639435
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For a disordered circular quantum dot of radius (formula presented), one has (formula presented), see
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For a disordered circular quantum dot of radius (formula presented), one has (formula presented), seeK.M. Frahm and J.-L. Pichard, J. Phys. I 5, 847 (1995).
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(1995)
J. Phys. I
, vol.5
, pp. 847
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Frahm, K.M.1
Pichard, J.-L.2
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